I have successfully computed thermal inertia on a seasonal basis using THEMIS data for a region in Mars which I found to be sinusoidally varying, peaking at Ls = 250-270 and dipping at Ls = 90-110. What may be the cause for this variation and how do I substantiate my conclusion with other data like Curiosity?
I found this old paper of JPL which talks about the application of thermal inertia in material identification. I thought it would be helpful even though it mentions the diurnal heating cycle on Earth. Of course THEMIS ASU webpage has pertinent information.
http://gis.ess.washington.edu/keck/Publications/Use%20of%20thermal-inertia%20properties%20for%20material%20identification.pdf
https://themis.asu.edu/projects
Thank you Mr. James. However, the paper gives a very vague method of identification of minerals using thermal inertia. It does not possess any scientific approach based on a physical or mathematical background. I am looking for possible applications of thermal inertia which can be substantiated by necessary auxiliary data and processing.
Like I said the paper is old (nearly four decades!). But to say that 'it does not possess any scientific approach based on a physical or mathematical background' would be unfair I think, especially given the understanding in the late 70's. If I were you, I would sift through existing literature on the topic and get in touch with subject matter experts like Phillip Christensen to take the discussion further. In any case, good luck with your research.
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